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https://doi.org/10.1...arrow_drop_down
https://doi.org/10.1007/109950...
Part of book or chapter of book . 2006 . Peer-reviewed
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https://dx.doi.org/10.1007/109...
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Conference object . 2005
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High Redshift Lyman Break Galaxies

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Other literature type , Conference object 05 Jan 2006 English Publisher:Springer Science and Business Media LLC
Authors: Lehnert, M.; Bremer, M.;

doi: 10.1007/10995020_3

handle: 11858/00-001M-0000-0011-DC41-3

High Redshift Lyman Break Galaxies

Abstract

Two of the most outstanding issues in modern astrophysics are what reionized the Universe and how did the first objects form. Observations of galaxies selected through the Lyman-Break technique indicate that UV photon output at the end of reionization was dominated by relatively faint low mass galaxies and not AGN.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
1
Average
Average
Average
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